- Abstract:
-
We consider the problem of self-regulated heating and cooling in galaxy clusters and the implications for cluster magnetic fields and turbulence. Viscous heating of a weakly collisional magnetised plasma is regulated by the pressure anisotropy with respect to the local direction of the magnetic field. The intracluster medium is a high-beta plasma, where pressure anisotropies caused by the turbulent stresses and the consequent local changes in the magnetic field will trigger very fast microsca...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1111/j.1365-2966.2010.17621.x
-
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- Journal:
- MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Volume:
- 410
- Issue:
- 4
- Pages:
- 2446-2457
- Publication date:
- 2010-03-13
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:794d1a61-c907-49b6-be0d-6efb9bebe032
- Source identifiers:
-
120290
- Local pid:
- pubs:120290
- Language:
- English
- Keywords:
- Copyright date:
- 2010
- Notes:
-
12 pages, 4 figures, 1 table; substantial revision with essential new
content
Journal article
A thermally stable heating mechanism for the intracluster medium: turbulence, magnetic fields and plasma instabilities
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